Lithium in Large Magellanic Cloud carbon stars

D. Hatzidimitriou*, D. H. Morgan, R. D. Cannon, B. F.W. Croke

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    15 Citations (Scopus)

    Abstract

    19 carbon stars that show lithium enrichment in their atmospheres have been discovered among a sample of 674 carbon stars in the Large Magellanic Cloud. Six of the Li-rich carbon stars are of the J type, i.e. they show strong 13C isotopic features. No super-Li-rich carbon stars were found. The incidence of lithium enrichment among carbon stars in the LMC is much rarer than in the Galaxy, and about five times more frequent among J-type than among N-type carbon stars. The bolometric magnitudes of the Li-rich carbon stars range between -3.3 and -5.7. Existing models of Li-enrichment via the hot bottom burning process fail to account for all of the observed properties of the Li-enriched stars studied here.

    Original languageEnglish
    Pages (from-to)1290-1298
    Number of pages9
    JournalMonthly Notices of the Royal Astronomical Society
    Volume341
    Issue number4
    DOIs
    Publication statusPublished - 1 Jun 2003

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